Diagnostics of non-thermal distribution from solar flares spectra - RESIK

Details Diagnostics of non-thermal distribution from solar flares spectra - RESIK Diagnostics of non-thermal distribution from solar flares spectra - RESIK

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010nspm.conf...77k&link_type=abstract

Proceedings of the 20th National Solar Physics Meeting, held 31 May - 4 June, 2010 in Papradno, Slovakia, p. 77

Physics

Scientific paper

Solar flares spectra observed by X-ray spectrometers RESIK and RHESSI made possible detecting and diagnosing non-thermal effects in the flare plasma in energy range from 2 keV to several tens of keV. Based on previous studies we have assumed that the core of a non-thermal distribution behaves like a so-called n-distribution mixed with a thermal component, and its high-energy tail can be described by a power-law relation. We used two different diagnostics: spectral lines ratia (RESIK) and a raw target model with a thermal component (RHESSI) to obtain parameters of these parts of the free electron 'model' distribution.

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